CWNU 4861

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UTI:
UCC Trust Index

C_N C_dens C_C3 C_lit C_dup
0.0 0.03 0.12 0.0 0.88
C3
N_50
r_50
DC 13 5.7
Summary

CWNU 4861 is a sparse, very loose object of very low C3 quality. It is located at a large distance from the Sun, below the mid-plane. It was recently reported in the literature.

This is very likely a unique object, which shares a small percentage of members with at least one previously reported entry.

Warning: contains less than 25 stars with P>0.5 estimated.

Warning: the low UTI value and no obvious signs of duplication (C_dup=0.88) indicates that this is quite probably an asterism, moving group, or artifact, and not a real open cluster.

Search object in SciX | Simbad

Positions

Reference RA DEC Plx pmRA pmDE Rv
He et al. (2023) 163.285 -65.542 0.189 -5.776 2.434 –
           
UCC 163.365 -65.538 0.184 -5.826 2.419 24.127
Galactocentric position Galactocentric position diagram

How are the galactocentric plots generated?

Search coordinates in CDS | Simbad

Estimated members

CWNU 4861 UCC

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Fundamental parameters

Reference Values
He et al. (2023) A0=1.25, m-M=13.55, logA=9.8

Search coordinates in Bayestar19

Cluster region map

Objects with shared members

Cluster % RA DEC Plx pmRA pmDE Rv UTI
HSC 2409 12.0 163.54 -65.66 0.14 -5.56 2.48 51.29 0.09